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The ARIEL space mission

  • Enzo Pascale
  • , Naidu Bezawada
  • , Joanna Barstow
  • , Jean Philippe Beaulieu
  • , Neil Bowles
  • , Vincent Coudé Du Foresto
  • , Athena Coustenis
  • , Leen Decin
  • , Pierre Drossart
  • , Paul Eccleston
  • , Therese Encrenaz
  • , Francois Forget
  • , Matt Griffin
  • , Manuel Güdel
  • , Paul Hartogh
  • , Astrid Heske
  • , Pierre Olivier Lagage
  • , Jeremy Leconte
  • , Pino Malaguti
  • , Giusi Micela
  • Kevin Middleton, Michiel Min, Andrea Moneti, Juan Carlos Morales, Lorenzo Mugnai, Marc Ollivier, Emanuele Pace, Andreas Papageorgiou, Goran Pilbratt, Ludovic Puig, Miroslaw Rataj, Tom Ray, Ignasi Ribas, Marco Rocchetto, Subhajit Sarkar, Franck Selsis, William Taylor, Jonathan Tennyson, Giovanna Tinetti, Diego Turrini, Bart Vandenbussche, Olivia Venot, Ingo P. Waldmann, Paulina Wolkenberg, Gillian Wright, Maria Rosa Zapatero Osorio, Tiziano Zingales
  • University of Rome
  • Cardiff University
  • Royal Observatory
  • University College London
  • Sorbonne Université
  • University of Oxford
  • Sorbonne Univ.
  • KU Leuven
  • RAL Space
  • University of Vienna
  • MPI for Solar System Research
  • ESTEC - European Space Research and Technology Centre
  • Univ. Bordeaux
  • Université Paris-Diderot
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
  • Istituto di Astrofisica e Planetologia Spaziali (IAPS)
  • SRON - Netherlands Institute for Space Research
  • Dublin Institute for Advanced Studies
  • University of Sheffield
  • Lab. Interuniversitaire Systemes
  • Polish Academy of Sciences
  • CAB
  • University of Florence

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Résumé

The Atmospheric Remote-Sensing Infrared Exoplanet Large-survey, ARIEL, has been selected to be the next M4 space mission in the ESA Cosmic Vision programme. From launch in 2028, and during the following 4 years of operation, ARIEL will perform precise spectroscopy of the atmospheres of about 1000 known transiting exoplanets using its metre-class telescope, a three-band photometer and three spectrometers that will cover the 0.5 μm to 7.8 μm region of the electromagnetic spectrum. The payload is designed to perform primary and secondary transit spectroscopy, and to measure spectrally resolved phase curves with a stability of < 100 ppm (goal 10 ppm). Observing from an L2 orbit, ARIEL will provide the first statistically significant spectroscopic survey of hot and warm planets. These are an ideal laboratory in which to study the chemistry, the formation and the evolution processes of exoplanets, to constrain the thermodynamics, composition and structure of their atmospheres, and to investigate the properties of the clouds.

langue originaleAnglais
titreSpace Telescopes and Instrumentation 2018
Sous-titreOptical, Infrared, and Millimeter Wave
rédacteurs en chefGiovanni G. Fazio, Howard A. MacEwen, Makenzie Lystrup
EditeurSPIE
ISBN (imprimé)9781510619494
Les DOIs
étatPublié - 1 janv. 2018
EvénementSpace Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave - Austin, États-Unis
Durée: 10 juin 201815 juin 2018

Série de publications

NomProceedings of SPIE - The International Society for Optical Engineering
Volume10698
ISSN (imprimé)0277-786X
ISSN (Electronique)1996-756X

Une conférence

Une conférenceSpace Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
Pays/TerritoireÉtats-Unis
La villeAustin
période10/06/1815/06/18

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